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通过约束实现自贝叶斯像差去除用于超冷原子显微镜

Self-Bayesian aberration removal via constraints for ultracold atom microscopy.

作者信息

Altuntaş Emine, Spielman I B

机构信息

Joint Quantum Institute, National Institute of Standards and Technology, and University of Maryland, Gaithersburg, Maryland 20899, USA.

出版信息

Phys Rev Res. 2021 Oct;3(4). doi: 10.1103/physrevresearch.3.043087.

Abstract

High-resolution imaging of ultracold atoms typically requires custom high numerical aperture (NA) optics, as is the case for quantum gas microscopy. These high NA objectives involve many optical elements, each of which contributes to loss and light scattering, making them unsuitable for quantum backaction limited "weak" measurements. We employ a low-cost high NA aspheric lens as an objective for a practical and economical-although aberrated-high-resolution microscope to image Rb Bose-Einstein condensates. Here, we present a methodology for digitally eliminating the resulting aberrations that is applicable to a wide range of imaging strategies and requires no additional hardware. We recover nearly the full NA of our objective, thereby demonstrating a simple and powerful digital aberration correction method for achieving optimal microscopy of quantum objects. This reconstruction relies on a high-quality measure of our imaging system's even-order aberrations from density-density correlations measured with differing degrees of defocus. We demonstrate our aberration compensation technique using phase-contrast imaging, a dispersive imaging technique directly applicable to quantum backaction limited measurements. Furthermore, we show that our digital correction technique reduces the contribution of photon shot noise to density-density correlation measurements which would otherwise contaminate the desired quantum projection noise signal in weak measurements.

摘要

超冷原子的高分辨率成像通常需要定制的高数值孔径(NA)光学器件,量子气体显微镜就是这种情况。这些高NA物镜包含许多光学元件,每个元件都会导致损耗和光散射,因此不适合用于量子反作用限制的“弱”测量。我们使用低成本的高NA非球面透镜作为物镜,构建了一台实用且经济实惠(尽管存在像差)的高分辨率显微镜,用于对铷玻色 - 爱因斯坦凝聚体进行成像。在此,我们提出一种数字消除由此产生的像差的方法,该方法适用于广泛的成像策略,且无需额外硬件。我们恢复了物镜几乎全部的NA,从而展示了一种简单而强大的数字像差校正方法,可实现对量子物体的最佳显微镜观察。这种重建依赖于通过不同散焦程度下测量的密度 - 密度相关性对成像系统偶数阶像差的高质量测量。我们使用相衬成像展示了我们的像差补偿技术,相衬成像是一种直接适用于量子反作用限制测量的色散成像技术。此外,我们表明我们的数字校正技术减少了光子散粒噪声对密度 - 密度相关性测量的贡献,否则在弱测量中光子散粒噪声会污染所需的量子投影噪声信号。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ded4/9830780/ad1bde462a0c/nihms-1858633-f0001.jpg

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